astro.wikisort.org - Asteroid(120132) 2003 FY128, also written as (120132) 2003 FY128, is a trans-Neptunian object with a diameter of about 460 km.[4] It orbits the Sun at a distance of about 49.81 astronomical units.[3] It was discovered on 26 March 2003 by the NEAT program at the Palomar Observatory, California.
(120132) 2003 FY128 |
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Discovered by | NEAT |
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Discovery date | 26 March 2003 |
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MPC designation | (120132) 2003 FY128 |
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Alternative designations | none |
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Minor planet category | detached object[2] |
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Epoch 13 January 2016 (JD 2457400.5) |
Uncertainty parameter 3 |
Observation arc | 8159 days (22.34 yr) |
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Aphelion | 62.551 AU (9.3575 Tm) |
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Perihelion | 37.066 AU (5.5450 Tm) |
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Semi-major axis | 49.809 AU (7.4513 Tm) |
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Eccentricity | 0.25584 |
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Orbital period (sidereal) | 351.53 yr (128397 d) |
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Mean anomaly | 28.257° |
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Mean motion | 0° 0m 10.094s / day |
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Inclination | 11.757° |
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Longitude of ascending node | 341.68° |
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Argument of perihelion | 175.26° |
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Earth MOID | 36.0755 AU (5.39682 Tm) |
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Jupiter MOID | 31.6621 AU (4.73658 Tm) |
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Dimensions | 460±21 km[4] |
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Synodic rotation period | 8.54 h (0.356 d) |
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Geometric albedo | 0.079±0.010[4] |
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Absolute magnitude (H) | 4.8[3] |
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Classification
It is classified as a detached object by the Deep Ecliptic Survey (DES), since its orbit appears to be beyond the current control of Neptune.[2] Though, if Neptune migrated outward, there would have been a period when Neptune had a higher eccentricity.
References
- Lowe, Andrew. "(120132) 2003 FY128 Precovery Images". andrew-lowe.ca.
- Marc W. Buie (2006-04-02). "Orbit Fit and Astrometric record for 120132". SwRI (Space Science Department). Retrieved 2009-01-22.
- "JPL Small-Body Database Browser: 120132 (2003 FY128)" (last observation: 2006-04-02). Retrieved 7 April 2016.
- Santos-Sanz, P.; Lellouch, E.; Fornasier, S.; Kiss, C.; Pal, A.; Müller, T. G.; Vilenius, E.; Stansberry, J.; Mommert, M.; Delsanti, A.; Mueller, M.; Peixinho, N.; Henry, F.; Ortiz, J. L.; Thirouin, A.; Protopapa, S.; Duffard, R.; Szalai, N.; Lim, T.; Ejeta, C.; Hartogh, P.; Harris, A. W.; Rengel, M. (2012). ""TNOs are Cool": A survey of the trans-Neptunian region". Astronomy & Astrophysics. 541: A92. arXiv:1202.1481. Bibcode:2012A&A...541A..92S. doi:10.1051/0004-6361/201118541. S2CID 118600525.
External links
Dwarf planets |
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Asteroid belt | | |
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Plutinos | |
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Twotinos | |
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Cubewanos and other Kuiper belt | Consensus | |
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Possible (cubewanos) | |
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Possible (other) | |
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Scattered disc | |
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Category
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Trans-Neptunian objects |
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TNO classes |
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На других языках
[de] (120132) 2003 FY128
(120132) 2003 FY128 ist ein großes transneptunisches Objekt, das bahndynamisch als nahes oder erweitertes Scattered Disc Object (SDO oder DO) eingestuft wird. Aufgrund seiner Größe ist der Asteroid ein Zwergplanetenkandidat.
- [en] (120132) 2003 FY128
[ru] (120132) 2003 FY128
(120132) 2003 FY128 транснептуновый объект. Он был обнаружен в рамках программы NEAT, в Паломарской обсерватории, Калифорния.
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